most citedA fundamental limit to how close binary systems can get via stable mass transfer shapes the properties of binary black hole mergers

9 citations · 25 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2026★ 4 cited

Thermal-timescale accretion does not always yield critical rotation in mass gainers

Chen Wang, Mike Y. M. Lau, Xiang-Dong Li +7

Binary evolution plays a central role in producing rapidly rotating stars. Previous studies have shown that mass gainers in binaries can reach critical rotation after accreting onl…

astro-ph.SR2025

The formation of merging black holes via stable mass transfer in massive binary stars

Xiao-Tian Xu, Norbert Langer, Jakub Klencki +2

The vast majority of massive binary systems in the universe is evidently unsuited to produce merging binary black holes. However, several narrow evolutionary paths of isolated mass…

astro-ph.SR2025★ 7 cited

A comprehensive grid of massive binary evolution models for the Galaxy - Surface properties of post-mass transfer stars

Harim Jin, Norbert Langer, Andrea Ercolino +1

Massive stars often evolve in binary systems, in which binary interactions significantly affect their evolution. Massive stars in the Galaxy serve as valuable testbeds for this due…

astro-ph.HE2025★ 9 cited

A fundamental limit to how close binary systems can get via stable mass transfer shapes the properties of binary black hole mergers

Jakub Klencki, Philipp Podsiadlowski, Norbert Langer +4

Mass transfer in binary systems is the key process in the formation of various classes of objects, including merging binary black holes (BBHs) and neutron stars. Orbital evolution…

astro-ph.HE2025★ 5 cited

Evidence of polar and ultralow supernova kicks from the orbits of Be X-ray binaries

Ruggero Valli, Selma E. de Mink, Stephen Justham +7

Supernovae, the explosive deaths of massive stars, create heavy elements and form black holes and neutron stars. These compact objects often receive a velocity at formation, a "kic…